English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We briefly review our work about the polarized foreground contamination ofthe Cosmic Microwave Background maps. We start by summarizing the mainproperties of the polarized cosmological signal, resulting in "electric" (E)and "magnetic" (B) components of the polarization tensor field on the sky. Thenwe describe our present understanding of sub-degree anisotropies from Galacticsynchrotron and from extra-Galactic point sources. We discuss theircontamination of the cosmological E and B modes.Comment: six pages including 2 figures, to appear in S. Cecchini et al.,  Astrophysical Polarized Backgrounds, AIP Conf. Proceeding

Polarized foregrounds power spectra vs CMB